Presented By: Department of Physics
HEP-Astro Seminar | Methods and Challenges in Searches for Continuous Gravitational Wave Signals
Orion Sauter and Ansel Neunzert (U-M Physics)
Recently, LIGO has made great strides in detecting gravitational waves produced by the coalescence of black holes and neutron stars. Nonetheless, a major target of LIGO observations remains elusive: continuous waves from fast-spinning, galactic neutron stars. We outline a few of the techniques used to search for these signals, and detail the challenges such searches present.
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